The relation between the radio jet and the near-IR line emission in Seyfert galaxies

Details The relation between the radio jet and the near-IR line emission in Seyfert galaxies The relation between the radio jet and the near-IR line emission in Seyfert galaxies

Feb 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011iaus..275..172r&link_type=abstract

Jets at all Scales, Proceedings of the International Astronomical Union, IAU Symposium, Volume 275, p. 172-173

Astronomy and Astrophysics

Astronomy

Galaxies: Seyfert, Galaxies: Jets, Galaxies: Kinematics And Dynamics

Scientific paper

We used near-IR integral field spectroscopy, obtained with Gemini NIFS and GNIRS integral field units (IFUs), to map the ionized and molecular flux distributions and kinematics in the central few hundreds of parsecs of Seyfert galaxies. We conclude that the molecular gas emission can be considered a tracer of the feeding of the AGN, while the emission of the ionized gas a tracer of its feedback.

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